A dataset provided by the European Space Agency

Name OT1_rmeijeri_1
Title Gas excitation through black hole accretion and star formation in the centers of active galaxies.
URL

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DOI https://doi.org/10.5270/esa-mitjanj
Author European Space Agency
Description Stunning observations with SPIRE FTS of Mrk 231 have shown that CO lines are very bright up to J=13-12, and there is no sign of a decline in the CO Spectral Line Energy Distribution (SLED). Our SPIRE FTS spectra show that this is a common feature of AGN type galaxies. Therefore, we propose to observe a set of 4 very high-J CO line transitions using the PACS spectrometer, for 5 of these well studied proto-typical (Ultra-)Luminous Infrared Galaxies ((U)LIRGs) and one starburst galaxy. The question of the relative role and contribution of AGN to the far-infrared luminosities of local (U)LIRG systems has long been a problem in our understanding of the evolutionary path of these objects, and as well for the interpretation of deep far-infrared surveys.

Our SPIRE FTS and our ground-based CO line observations together with the PACS observations in this program will allow us, for the first time, to complete a full CO SLED for a set of (U)LIRGs. Combining this with our models of Photon Dominated Regions (PDRs) and X-ray Dominated Regions (XDRs), we will then be able to determine the physical state of the interstellar medium and estimate the starburst/AGN contribution to the total energetics of these systems.
Publication Hidden or missing outflows in highly obscured galaxy nuclei? . Falstad N. et al. . Astronomy & Astrophysics, Volume 623, id.A29, 10 pp. . 623 . 10.1051\/0004-6361\/201834586 . 2019A&A...623A..29F ,
Far-infrared Line Spectra of Active Galaxies from the Herschel/PACS Spectrometer: The Complete Database . Fernández-Ontiveros Juan Antonio et al. . The Astrophysical Journal Supplement Series, Volume 226, Issue 2, article id. 19, 26 pp. (2016). . 226 . 10.3847\/0067-0049\/226\/2\/19 . 2016ApJS..226...19F ,
Importance of radiative pumping for the excitation of the H2O submillimeter lines in galaxies . González-Alfonso Eduardo et al. . Astronomy and Astrophysics . null . null . 2022A&A...666L...3G ,
Instrument PACS_PacsRangeSpec_point
Temporal Coverage 2010-12-31T13:10:10Z/2012-08-24T07:39:09Z
Version SPG v14.2.0
Mission Description Herschel was launched on 14 May 2009! It is the fourth 'cornerstone' mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 µm range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/h®erschel/
Date Published 2013-02-24T07:03:21Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013, Gas Excitation Through Black Hole Accretion And Star Formation In The Centers Of Active Galaxies., SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-mitjanj